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Multipole Charge Conservation and Implications on Electromagnetic Radiation Published for SISSA by Springer Received: November 7, 2016 Revised: February 18, 2017 Accepted: June 7, 2017 Published: June 15, 2017 JHEP06(2017)080 Multipole charge conservation and implications on electromagnetic radiation Ali Seraj School of Physics, Institute for Research in Fundamental Sciences (IPM), P.O.Box 19395-5531, Tehran, Iran E-mail: ali [email protected] Abstract: It is shown that conserved charges associated with a specific subclass of gauge symmetries of Maxwell electrodynamics are proportional to the well known electric mul- tipole moments. The symmetries are residual gauge transformations surviving the Lorenz gauge, with nontrivial conserved charge at spatial infinity. These \Multipole charges" re- ceive contributions both from the charged matter and electromagnetic fields. The former is nothing but the electric multipole moment of the source. In a stationary configuration, there is a novel equipartition relation between the two contributions. The multipole charge, while conserved, can freely interpolate between the source and the electromagnetic field, and therefore can be propagated with the radiation. Using the multipole charge conserva- tion, we obtain infinite number of constraints over the radiation produced by the dynamics of charged matter. Keywords: Gauge Symmetry, Global Symmetries, Space-Time Symmetries ArXiv ePrint: 1610.02870 Open Access, c The Authors. https://doi.org/10.1007/JHEP06(2017)080 Article funded by SCOAP3. Contents 1 Introduction1 2 Gauge symmetries and conservation laws3 2.1 Charges in the covariant phase space3 2.2 Noether current5 2.3 Residual gauge symmetries and asymptotic symmetries6 JHEP06(2017)080 3 Residual gauge symmetries of Maxwell theory7 3.1 The nontrivial sector8 4 Stationary configurations 10 4.1 Electrostatics 11 4.1.1 Screening effect and equi-partition relation 12 4.1.2 Symplectic symmetries 12 4.2 Magnetostatics 13 5 Electrodynamics 14 5.1 Conservation 14 5.2 A preliminary example 14 5.3 Infinite constraints over radiation 16 6 Discussion 17 A Algebra of charges in covariant phase space 19 1 Introduction In her seminal paper, E. Noether established a profound link between the symmetries and constants of motion in the action formulation of particle or field theories [1]. This can also be rephrased in the Hamiltonian description where a symmetry can be associated with a function over the phase space which commutes with the Hamiltonian of the system and also generates the symmetry transformation through the Poisson bracket. These results continue to hold in the quantum theory if the symmetry is anomaly free. Dividing symmetries of a theory into global or local, the above theorem is usually supposed to be restricted to the former. Local (gauge) symmetries, on the other hand, are considered in the Noether's second theorem (also discussed in [1]) which states that the existence of local symmetries, implies a set of constraints for the theory, usually known as Bianchi identities. { 1 { However, simultaneous implementation of both of the above Noether theorems leads to the association of a conserved charge to a local (gauge) symmetry as well [2{4]. The key result in this case, is that the charges can be formulated as surface (codimension 2) integrals, instead of volume (codimension 1) integrals. Accordingly, if the fields drop fast enough near the boundary, the charges associated with local symmetries would vanish. While this is usually presumed in quantum field theory, it is not the case in many examples of physical interest. A more relaxed boundary condition on gauge fields, can make the surface integral charges nonvanishing. However, one should make sure that such relaxation does not lead to divergent charges. The \large gauge transformations" allowed by the relaxed boundary conditions having nonvanishing charges, form a closed algebra called the JHEP06(2017)080 asymptotic symmetry algebra. On the other hand, one may put the boundary conditions on gauge invariant quantities like the field strength, instead of gauge field itself. This can be more physical, since the observable quantities are gauge invariant. Such boundary condition impose no restriction on the allowed gauge transformations. However, still a subclass of gauge transformations can be singled out by choosing a gauge condition instead of a boundary condition. While the gauge fixing condition kills most of the gauge redundancies, it allows for residual gauge transformations respecting a given gauge condition. Such viewpoint was stressed in [5{8]. In this paper, we will follow this approach and show that a subclass of residual gauge transformations can be associated with nontrivial conserved charges. In the context of Maxwell electrodynamics, we will show that such conserved quantities have a very nice interpretation in terms of electric multipole moments. Multipole moments in electrodynamics are obviously not conserved. For example a point charge located at origin of space has only monopole moment, while if it starts to leave the origin, it will obtain dipole and higher moments. However, we will show that if a \soft multipole charge" is attributed to the electromagnetic field, the total multipole charge composed of hard and soft pieces will be a conserved quantity. Interestingly, it turns out that this charge is nothing but the conserved charge associated with residual symmetries of electrodynamics. The multipole charge can freely interpolate between the charged matter and the electromagnetic field. The organization of the paper is as follows. In section2 we derive in a systematic way, the conserved charges associated with nontrivial gauge symmetries, using the covariant phase space method. Those who are not interested in the details of the derivation can easily jump to (2.18) and (2.20).1 In section3 we determine the residual symmetries as the physical subset of U(1) gauge transformations of Maxwell theory. Then in section4 we compute -in an electrostatic configuration- the charges associated with these symmetries and show our main result relating the charges and electric multipole moments. In section5 we discuss electrodynamics and show how the above conservation laws put constraints on the radiation. We conclude in section6 . An appendix is devoted to the Poisson bracket of charges over the covariant phase space. 1Although in Maxwell theory, these results can also be obtained by the usual Noether's approach, but in general the Hamiltinian approaches are preferred since e.g. in gravity the Noether charge is only a part of the correct charge [3, 15]. { 2 { 2 Gauge symmetries and conservation laws We consider the theory of Maxwell electrodynamics sourced by an arbitrary charged matter field. We choose the natural units in which "0 = µ0 = c = 1 and the Largrangian takes the form 1 L = − F F µν − jµA + L ; (2.1) 4 µν µ matter µ where Fµν = @[µAν] ≡ @µAν − @νAµ is the field strength, and the current j must be conserved JHEP06(2017)080 µ @µj = 0 : (2.2) Variation with respect to Aµ leads to the Maxwell field equations µν ν @µF = j : (2.3) In the next section, we give a systematic approach to compute the charges associated with gauge symmetries. 2.1 Charges in the covariant phase space In order to be able to study the conservation laws associated with gauge symmetries, one can use the Hamiltonian formulation of gauge theories [9{12] which is well established. However, this has the drawback that it breaks the manifest covariance of the theory, and potentially leads to cumbersome expressions. Instead, one can use a pretty mathematical construction called the \covariant phase space" to study gauge symmetries and associated conserved charges [2,3 , 13{16] (see also [17] for a review). This is the setup we use in this paper. To start, one needs to define a symplectic form on the space of field configurations. The symplectic form can then be used to define a Poisson bracket between functionals (of dynamical fields). Moreover, one can associate a Hamiltonian to each gauge symmetry, which generates that gauge transformation through the Poisson bracket. The on-shell value of the Hamiltonian will define the charge of that gauge symmetry. According to the action principle, the on-shell variation of the Lagrangian is by con- struction a total derivative δL ≈ dΘ(δ ) ; (2.4) where L is the Lagrangian as a top form, and stands collectively for all dynamical fields in the theory (in our case the gauge field Aµ and the matter field φ). Taking another antisymmetric variation of Θ defines the symplectic current ! (as a d−1 form of spacetime and a two form over the phase space) !( ; δ1 ; δ2 ) = δ1Θ(δ2 ) − δ2Θ(δ1 ) : (2.5) { 3 { The pre-symplectic form Ω( ; δ1 ; δ2 ) is defined through the symplectic current ! Z Ω( ; δ1 ; δ2 ) = !( ; δ1 ; δ2 ) ; (2.6) Σ over a spacelike hypersurface Σ in spacetime. A gauge theory involves local symmetry transformations of the form ! + δλ where λ(x) is a local function (or tensor) that parametrizes the gauge transformation. The Hamiltonian associated to a symmetry transformation ! + δλ (either local or global) is then defined through JHEP06(2017)080 δHλ = Ω( ; δ ; δλ ) : (2.7) It is proved [2,3 ] that for a gauge transformation in a gauge invariant theory one has !( ; δ ; δλ ) = d kλ( ; δ ) ; (2.8) that is the symplectic current contracted with a gauge transformation is necessarily an exact form. Accordingly I δHλ = kλ( ; δ ) : (2.9) @Σ Therefore one finds the important result that the conserved charge associated with a gauge symmetry is given by a co-dimension 2 integral. Meanwhile the conserved charge of a global symmetry is given by a volume integral. This explains why the electric charge is given by the Gauss' surface integral. On the other hand it shows why energy and angular momenta are given by volume integrals in Special Relativity (where Lorentz symmetries are global) while in General Relativity, where diffeomorphisms are local symmetries, similar quantities are given by surface integrals.
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